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تسجيل مستخدم جديدThe radial Teukolsky equation for Kerr-Newman-de Sitter geometry: Revisited
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M. Hortacsu
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We use Heun type solutions given in cite{Suzuki} for the radial Teukolsky equation, written in the background metric of the Kerr-Newman-de Sitter geometry, to calculate the quasinormal frequencies for polynomial solutions and the reflection coefficient for waves coming from the de Sitter horizon and reflected at the outer horizon of the black hole.
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